Superradiant interactions of cosmic noise
APA
Galanis, M. (2024). Superradiant interactions of cosmic noise. Perimeter Institute. https://pirsa.org/24090187
MLA
Galanis, Marios. Superradiant interactions of cosmic noise. Perimeter Institute, Sep. 24, 2024, https://pirsa.org/24090187
BibTex
@misc{ pirsa_PIRSA:24090187, doi = {10.48660/24090187}, url = {https://pirsa.org/24090187}, author = {Galanis, Marios}, keywords = {Particle Physics}, language = {en}, title = {Superradiant interactions of cosmic noise}, publisher = {Perimeter Institute}, year = {2024}, month = {sep}, note = {PIRSA:24090187 see, \url{https://pirsa.org}} }
In this talk I will do three things. First, I will outline the conditions under which the interaction rate of inelastic processes with a system consisting of N targets scales as N^2. Second, I will present computations of interaction rates for several weakly interacting particles, including the Cosmic Neutrino Background and QCD axion dark matter, and will explain the underlying physics. Third, I will introduce new quantum observables that do not rely on net energy transfer, but can still extract these N^2 effects. This talk will not address a concrete experimental proposal, but the effects presented may point to a new class of table-top and ultra-low threshold particle detectors.